A CO-rich merger shaping a powerful and hyperluminous infrared radio galaxy at z = 2: the Dragonfly Galaxy
A galaxy populations study of a radio-selected protocluster at z ~ 3.1
CO(1-0) survey of high-z radio galaxies: alignment of molecular halo gas with distant radio sources
CO Survey of High-z Radio Galaxies, Revisited with the Atacama Large Millimeter/submillimeter Array: Jet-Cloud Alignments and Synchrotron Brightening by Molecular Gas in the Circumgalactic Environment
OIII emitters in the field of the MRC0316-257 protocluster
On the X-ray emission of z ~2 radio galaxies: IC scattering of the CMB and no evidence for fully-formed potential wells
Properties of Lya emitters around the radio galaxy MRC 0316 257,
The Dragonfly Galaxy. II. ALMA unveils a triple merger and gas exchange in a hyper-luminous radio galaxy at z = 2
The impact of satellite trails on Hubble Space Telescope observations
The realm of the galaxy protoclusters. A review
Instrument
ACS, ACS/WFC, WFPC2, WFPC2/PC
Temporal Coverage
1999-10-19T10:32:13Z/2002-07-18T22:53:16Z
Version
1.0
Mission Description
Launched in 1990, the NASA/ESA Hubble Space Telescope remains the premier UV and visible light telescope in orbit. With well over 1.6 million observations from 10 different scientific instruments, the ESA Hubble Science Archive is a treasure trove of astronomical data to be exploited.
European Space Agency, Miley comma George K., 2003, 'Morphology of the most massive galaxies in the early universe', 1.0, European Space Agency, https://doi.org/10.5270/esa-88k8vcj
